Neural Network Forecast of the Sunspot Butterfly Diagram

被引:42
作者
Covas, Eurico [1 ]
Peixinho, Nuno [1 ]
Fernandes, Joao [1 ,2 ]
机构
[1] Univ Coimbra, Geophys & Astron Observ, CITEUC Ctr Earth & Space Sci Res, P-3040004 Coimbra, Portugal
[2] Univ Coimbra, Dept Math, P-3001454 Coimbra, Portugal
关键词
Sunspots; Statistics; Solar cycle; Observations; MAGNETIC-FIELD; CYCLE; PREDICTION; CHAOS; SUN; RECONSTRUCTION; AA;
D O I
10.1007/s11207-019-1412-z
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using neural networks as a prediction method, we attempt to demonstrate that forecasting of the Sun's sunspot time series can be extended to the spatio-temporal case. We employ this machine-learning method to forecast not only in time but also in space (in this case, latitude) on a spatio-temporal dataset representing the solar sunspot diagram extending to a total of 142 years. The analysis shows that this approach seems to be able to reconstruct the overall qualitative aspects of the spatial-temporal series, namely the overall shape and amplitude of the latitude and time pattern of sunspots. This is, as far as we are aware, the first time that neural networks have been used to forecast the Sun's sunspot butterfly diagram, and although the results are limited in the quantitative prediction aspects, it points to the way to use the full spatio-temporal series as opposed to just the time series for machine-learning approaches to forecasting. Additionally, we use the method to predict that the upcoming Cycle 25 maximum sunspot number will be around R25=57 +/- 17. This implies a very weak cycle and, in fact, the weakest cycle on record.
引用
收藏
页数:15
相关论文
共 79 条
[1]  
Abarbanel H.D., 1996, Physics Today, V49, P86, DOI DOI 10.1063/1.881528
[2]   Extreme Value Theory and the New Sunspot Number Series [J].
Acero, F. J. ;
Carrasco, V. M. S. ;
Gallego, M. C. ;
Garcia, J. A. ;
Vaquero, J. M. .
ASTROPHYSICAL JOURNAL, 2017, 839 (02)
[3]  
Altmann, 1986, PSYCHOLINGUISTICS
[4]  
[Anonymous], 2017, ARXIV E PRINTS
[5]  
[Anonymous], 1990, Readings Speech Recognit, DOI DOI 10.1016/B978-0-08-051584-7.50037-1
[6]  
[Anonymous], 2018, ARXIV E PRINTS
[7]   The Butterfly Diagram in the Eighteenth Century [J].
Arlt, R. .
SOLAR PHYSICS, 2009, 255 (01) :143-153
[8]   Solar Activity in the Past and the Chaotic Behaviour of the Dynamo [J].
Arlt, Rainer ;
Weiss, Nigel .
SPACE SCIENCE REVIEWS, 2014, 186 (1-4) :525-533
[9]   Transverse instability for non-normal parameters [J].
Ashwin, P ;
Covas, E ;
Tavakol, R .
NONLINEARITY, 1999, 12 (03) :563-577
[10]   An active sun throughout the Maunder Minimum [J].
Beer, J ;
Tobias, S ;
Weiss, N .
SOLAR PHYSICS, 1998, 181 (01) :237-249